CEERS Key Paper. VIII. Emission-line Ratios from NIRSpec and NIRCam Wide-Field Slitless Spectroscopy at z < 2

We use James Webb Space Telescope Near-Infrared Camera Wide Field Slitless Spectroscopy (NIRCam WFSS) and the Near-Infrared spectrograph (NIRSpec) in the Cosmic Evolution Early Release survey to measure rest-frame optical emission-line ratios of 155 galaxies at z < 2. The blind NIRCam grism obse...
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Autor*in:	Bren E. Backhaus [verfasserIn] Jonathan R. Trump [verfasserIn] Nor Pirzkal [verfasserIn] Guillermo Barro [verfasserIn] Steven L. Finkelstein [verfasserIn] Pablo Arrabal Haro [verfasserIn] Raymond C. Simons [verfasserIn] Jessica Wessner [verfasserIn] Nikko J. Cleri [verfasserIn] Micaela B. Bagley [verfasserIn] Michaela Hirschmann [verfasserIn] David C. Nicholls [verfasserIn] Mark Dickinson [verfasserIn] Jeyhan S. Kartaltepe [verfasserIn] Casey Papovich [verfasserIn] Dale D. Kocevski [verfasserIn] Anton M. Koekemoer [verfasserIn] Laura Bisigello [verfasserIn] Anne E. Jaskot [verfasserIn] Ray A. Lucas [verfasserIn] Intae Jung [verfasserIn] Stephen M. Wilkins [verfasserIn] L. Y. Aaron Yung [verfasserIn] Henry C. Ferguson [verfasserIn] Adriano Fontana [verfasserIn] Andrea Grazian [verfasserIn] Norman A. Grogin [verfasserIn] Lisa J. Kewley [verfasserIn] Allison Kirkpatrick [verfasserIn] Jennifer M. Lotz [verfasserIn] Laura Pentericci [verfasserIn] Pablo G. Pérez-González [verfasserIn] Swara Ravindranath [verfasserIn] Rachel S. Somerville [verfasserIn] Guang Yang [verfasserIn] Benne W. Holwerda [verfasserIn] Peter Kurczynski [verfasserIn] Nimish P. Hathi [verfasserIn] Caitlin Rose [verfasserIn] Kelcey Davis [verfasserIn]

Format:	E-Artikel
Sprache:	Englisch

Erschienen:	2024

Schlagwörter:	Emission line galaxies Galaxy evolution Galaxies Active galaxies

Übergeordnetes Werk:	In: The Astrophysical Journal - IOP Publishing, 2022, 962(2024), 2, p 195
Übergeordnetes Werk:	volume:962 ; year:2024 ; number:2, p 195

Links:	Link aufrufen Link aufrufen Link aufrufen Journal toc

DOI / URN:	10.3847/1538-4357/ad1520

Katalog-ID:	DOAJ100792480

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245	1	0	\|a CEERS Key Paper. VIII. Emission-line Ratios from NIRSpec and NIRCam Wide-Field Slitless Spectroscopy at z < 2
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520			\|a We use James Webb Space Telescope Near-Infrared Camera Wide Field Slitless Spectroscopy (NIRCam WFSS) and the Near-Infrared spectrograph (NIRSpec) in the Cosmic Evolution Early Release survey to measure rest-frame optical emission-line ratios of 155 galaxies at z < 2. The blind NIRCam grism observations include a sample of galaxies with bright emission lines that were not observed on the NIRSpec masks. We study the changes of the H α , [O III ]/H β , and [Ne III ]/[O II ] emission lines in terms of redshift by comparing to lower-redshift SDSS, CLEAR, and MOSDEF samples. We find a significant (<3 σ ) correlation between [O III ]/H β with redshift, while [Ne III ]/[O II ] has a marginal (2 σ ) correlation with redshift. We compare [O III ]/H β and [Ne III ]/[O II ] to stellar mass and H β SFR. We find that both emission-line ratios have a correlation with H β SFR and an anticorrelation with stellar mass across the redshifts 0 < z < 9. Comparison with MAPPINGS V models indicates that these trends are consistent with lower metallicity and higher ionization in low-mass and high-SFR galaxies. We additionally compare to IllustrisTNG predictions and find that they effectively describe the highest [O III ]/H β ratios observed in our sample, without the need to invoke MAPPINGS models with significant shock ionization components.
650		4	\|a Emission line galaxies
650		4	\|a Galaxy evolution
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650		4	\|a Active galaxies
653		0	\|a Astrophysics
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700	0		\|a Nor Pirzkal \|e verfasserin \|4 aut
700	0		\|a Guillermo Barro \|e verfasserin \|4 aut
700	0		\|a Steven L. Finkelstein \|e verfasserin \|4 aut
700	0		\|a Pablo Arrabal Haro \|e verfasserin \|4 aut
700	0		\|a Raymond C. Simons \|e verfasserin \|4 aut
700	0		\|a Jessica Wessner \|e verfasserin \|4 aut
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700	0		\|a Micaela B. Bagley \|e verfasserin \|4 aut
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700	0		\|a David C. Nicholls \|e verfasserin \|4 aut
700	0		\|a Mark Dickinson \|e verfasserin \|4 aut
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700	0		\|a Casey Papovich \|e verfasserin \|4 aut
700	0		\|a Dale D. Kocevski \|e verfasserin \|4 aut
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700	0		\|a Anne E. Jaskot \|e verfasserin \|4 aut
700	0		\|a Ray A. Lucas \|e verfasserin \|4 aut
700	0		\|a Intae Jung \|e verfasserin \|4 aut
700	0		\|a Stephen M. Wilkins \|e verfasserin \|4 aut
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700	0		\|a Norman A. Grogin \|e verfasserin \|4 aut
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700	0		\|a Allison Kirkpatrick \|e verfasserin \|4 aut
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700	0		\|a Nimish P. Hathi \|e verfasserin \|4 aut
700	0		\|a Caitlin Rose \|e verfasserin \|4 aut
700	0		\|a Kelcey Davis \|e verfasserin \|4 aut
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allfields	10.3847/1538-4357/ad1520 doi (DE-627)DOAJ100792480 (DE-599)DOAJe9f61abcfafa4e92872ba38af1d4f744 DE-627 ger DE-627 rakwb eng QB460-466 Bren E. Backhaus verfasserin aut CEERS Key Paper. VIII. Emission-line Ratios from NIRSpec and NIRCam Wide-Field Slitless Spectroscopy at z < 2 2024 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier We use James Webb Space Telescope Near-Infrared Camera Wide Field Slitless Spectroscopy (NIRCam WFSS) and the Near-Infrared spectrograph (NIRSpec) in the Cosmic Evolution Early Release survey to measure rest-frame optical emission-line ratios of 155 galaxies at z < 2. The blind NIRCam grism observations include a sample of galaxies with bright emission lines that were not observed on the NIRSpec masks. We study the changes of the H α , [O III ]/H β , and [Ne III ]/[O II ] emission lines in terms of redshift by comparing to lower-redshift SDSS, CLEAR, and MOSDEF samples. We find a significant (<3 σ ) correlation between [O III ]/H β with redshift, while [Ne III ]/[O II ] has a marginal (2 σ ) correlation with redshift. We compare [O III ]/H β and [Ne III ]/[O II ] to stellar mass and H β SFR. We find that both emission-line ratios have a correlation with H β SFR and an anticorrelation with stellar mass across the redshifts 0 < z < 9. Comparison with MAPPINGS V models indicates that these trends are consistent with lower metallicity and higher ionization in low-mass and high-SFR galaxies. We additionally compare to IllustrisTNG predictions and find that they effectively describe the highest [O III ]/H β ratios observed in our sample, without the need to invoke MAPPINGS models with significant shock ionization components. Emission line galaxies Galaxy evolution Galaxies Active galaxies Astrophysics Jonathan R. Trump verfasserin aut Nor Pirzkal verfasserin aut Guillermo Barro verfasserin aut Steven L. Finkelstein verfasserin aut Pablo Arrabal Haro verfasserin aut Raymond C. Simons verfasserin aut Jessica Wessner verfasserin aut Nikko J. Cleri verfasserin aut Micaela B. Bagley verfasserin aut Michaela Hirschmann verfasserin aut David C. Nicholls verfasserin aut Mark Dickinson verfasserin aut Jeyhan S. Kartaltepe verfasserin aut Casey Papovich verfasserin aut Dale D. Kocevski verfasserin aut Anton M. Koekemoer verfasserin aut Laura Bisigello verfasserin aut Anne E. Jaskot verfasserin aut Ray A. Lucas verfasserin aut Intae Jung verfasserin aut Stephen M. Wilkins verfasserin aut L. Y. Aaron Yung verfasserin aut Henry C. Ferguson verfasserin aut Adriano Fontana verfasserin aut Andrea Grazian verfasserin aut Norman A. Grogin verfasserin aut Lisa J. Kewley verfasserin aut Allison Kirkpatrick verfasserin aut Jennifer M. Lotz verfasserin aut Laura Pentericci verfasserin aut Pablo G. Pérez-González verfasserin aut Swara Ravindranath verfasserin aut Rachel S. Somerville verfasserin aut Guang Yang verfasserin aut Benne W. Holwerda verfasserin aut Peter Kurczynski verfasserin aut Nimish P. Hathi verfasserin aut Caitlin Rose verfasserin aut Kelcey Davis verfasserin aut In The Astrophysical Journal IOP Publishing, 2022 962(2024), 2, p 195 (DE-627)269019219 (DE-600)1473835-1 15384357 nnns volume:962 year:2024 number:2, p 195 https://doi.org/10.3847/1538-4357/ad1520 kostenfrei https://doaj.org/article/e9f61abcfafa4e92872ba38af1d4f744 kostenfrei https://doi.org/10.3847/1538-4357/ad1520 kostenfrei https://doaj.org/toc/1538-4357 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2014 GBV_ILN_2088 GBV_ILN_2522 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 962 2024 2, p 195
spelling	10.3847/1538-4357/ad1520 doi (DE-627)DOAJ100792480 (DE-599)DOAJe9f61abcfafa4e92872ba38af1d4f744 DE-627 ger DE-627 rakwb eng QB460-466 Bren E. Backhaus verfasserin aut CEERS Key Paper. VIII. Emission-line Ratios from NIRSpec and NIRCam Wide-Field Slitless Spectroscopy at z < 2 2024 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier We use James Webb Space Telescope Near-Infrared Camera Wide Field Slitless Spectroscopy (NIRCam WFSS) and the Near-Infrared spectrograph (NIRSpec) in the Cosmic Evolution Early Release survey to measure rest-frame optical emission-line ratios of 155 galaxies at z < 2. The blind NIRCam grism observations include a sample of galaxies with bright emission lines that were not observed on the NIRSpec masks. We study the changes of the H α , [O III ]/H β , and [Ne III ]/[O II ] emission lines in terms of redshift by comparing to lower-redshift SDSS, CLEAR, and MOSDEF samples. We find a significant (<3 σ ) correlation between [O III ]/H β with redshift, while [Ne III ]/[O II ] has a marginal (2 σ ) correlation with redshift. We compare [O III ]/H β and [Ne III ]/[O II ] to stellar mass and H β SFR. We find that both emission-line ratios have a correlation with H β SFR and an anticorrelation with stellar mass across the redshifts 0 < z < 9. Comparison with MAPPINGS V models indicates that these trends are consistent with lower metallicity and higher ionization in low-mass and high-SFR galaxies. We additionally compare to IllustrisTNG predictions and find that they effectively describe the highest [O III ]/H β ratios observed in our sample, without the need to invoke MAPPINGS models with significant shock ionization components. Emission line galaxies Galaxy evolution Galaxies Active galaxies Astrophysics Jonathan R. Trump verfasserin aut Nor Pirzkal verfasserin aut Guillermo Barro verfasserin aut Steven L. Finkelstein verfasserin aut Pablo Arrabal Haro verfasserin aut Raymond C. Simons verfasserin aut Jessica Wessner verfasserin aut Nikko J. Cleri verfasserin aut Micaela B. Bagley verfasserin aut Michaela Hirschmann verfasserin aut David C. Nicholls verfasserin aut Mark Dickinson verfasserin aut Jeyhan S. Kartaltepe verfasserin aut Casey Papovich verfasserin aut Dale D. Kocevski verfasserin aut Anton M. Koekemoer verfasserin aut Laura Bisigello verfasserin aut Anne E. Jaskot verfasserin aut Ray A. Lucas verfasserin aut Intae Jung verfasserin aut Stephen M. Wilkins verfasserin aut L. Y. Aaron Yung verfasserin aut Henry C. Ferguson verfasserin aut Adriano Fontana verfasserin aut Andrea Grazian verfasserin aut Norman A. Grogin verfasserin aut Lisa J. Kewley verfasserin aut Allison Kirkpatrick verfasserin aut Jennifer M. Lotz verfasserin aut Laura Pentericci verfasserin aut Pablo G. Pérez-González verfasserin aut Swara Ravindranath verfasserin aut Rachel S. Somerville verfasserin aut Guang Yang verfasserin aut Benne W. Holwerda verfasserin aut Peter Kurczynski verfasserin aut Nimish P. Hathi verfasserin aut Caitlin Rose verfasserin aut Kelcey Davis verfasserin aut In The Astrophysical Journal IOP Publishing, 2022 962(2024), 2, p 195 (DE-627)269019219 (DE-600)1473835-1 15384357 nnns volume:962 year:2024 number:2, p 195 https://doi.org/10.3847/1538-4357/ad1520 kostenfrei https://doaj.org/article/e9f61abcfafa4e92872ba38af1d4f744 kostenfrei https://doi.org/10.3847/1538-4357/ad1520 kostenfrei https://doaj.org/toc/1538-4357 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2014 GBV_ILN_2088 GBV_ILN_2522 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 962 2024 2, p 195
allfields_unstemmed	10.3847/1538-4357/ad1520 doi (DE-627)DOAJ100792480 (DE-599)DOAJe9f61abcfafa4e92872ba38af1d4f744 DE-627 ger DE-627 rakwb eng QB460-466 Bren E. Backhaus verfasserin aut CEERS Key Paper. VIII. Emission-line Ratios from NIRSpec and NIRCam Wide-Field Slitless Spectroscopy at z < 2 2024 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier We use James Webb Space Telescope Near-Infrared Camera Wide Field Slitless Spectroscopy (NIRCam WFSS) and the Near-Infrared spectrograph (NIRSpec) in the Cosmic Evolution Early Release survey to measure rest-frame optical emission-line ratios of 155 galaxies at z < 2. The blind NIRCam grism observations include a sample of galaxies with bright emission lines that were not observed on the NIRSpec masks. We study the changes of the H α , [O III ]/H β , and [Ne III ]/[O II ] emission lines in terms of redshift by comparing to lower-redshift SDSS, CLEAR, and MOSDEF samples. We find a significant (<3 σ ) correlation between [O III ]/H β with redshift, while [Ne III ]/[O II ] has a marginal (2 σ ) correlation with redshift. We compare [O III ]/H β and [Ne III ]/[O II ] to stellar mass and H β SFR. We find that both emission-line ratios have a correlation with H β SFR and an anticorrelation with stellar mass across the redshifts 0 < z < 9. Comparison with MAPPINGS V models indicates that these trends are consistent with lower metallicity and higher ionization in low-mass and high-SFR galaxies. We additionally compare to IllustrisTNG predictions and find that they effectively describe the highest [O III ]/H β ratios observed in our sample, without the need to invoke MAPPINGS models with significant shock ionization components. Emission line galaxies Galaxy evolution Galaxies Active galaxies Astrophysics Jonathan R. Trump verfasserin aut Nor Pirzkal verfasserin aut Guillermo Barro verfasserin aut Steven L. Finkelstein verfasserin aut Pablo Arrabal Haro verfasserin aut Raymond C. Simons verfasserin aut Jessica Wessner verfasserin aut Nikko J. Cleri verfasserin aut Micaela B. Bagley verfasserin aut Michaela Hirschmann verfasserin aut David C. Nicholls verfasserin aut Mark Dickinson verfasserin aut Jeyhan S. Kartaltepe verfasserin aut Casey Papovich verfasserin aut Dale D. Kocevski verfasserin aut Anton M. Koekemoer verfasserin aut Laura Bisigello verfasserin aut Anne E. Jaskot verfasserin aut Ray A. Lucas verfasserin aut Intae Jung verfasserin aut Stephen M. Wilkins verfasserin aut L. Y. Aaron Yung verfasserin aut Henry C. Ferguson verfasserin aut Adriano Fontana verfasserin aut Andrea Grazian verfasserin aut Norman A. Grogin verfasserin aut Lisa J. Kewley verfasserin aut Allison Kirkpatrick verfasserin aut Jennifer M. Lotz verfasserin aut Laura Pentericci verfasserin aut Pablo G. Pérez-González verfasserin aut Swara Ravindranath verfasserin aut Rachel S. Somerville verfasserin aut Guang Yang verfasserin aut Benne W. Holwerda verfasserin aut Peter Kurczynski verfasserin aut Nimish P. Hathi verfasserin aut Caitlin Rose verfasserin aut Kelcey Davis verfasserin aut In The Astrophysical Journal IOP Publishing, 2022 962(2024), 2, p 195 (DE-627)269019219 (DE-600)1473835-1 15384357 nnns volume:962 year:2024 number:2, p 195 https://doi.org/10.3847/1538-4357/ad1520 kostenfrei https://doaj.org/article/e9f61abcfafa4e92872ba38af1d4f744 kostenfrei https://doi.org/10.3847/1538-4357/ad1520 kostenfrei https://doaj.org/toc/1538-4357 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2014 GBV_ILN_2088 GBV_ILN_2522 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 962 2024 2, p 195
allfieldsGer	10.3847/1538-4357/ad1520 doi (DE-627)DOAJ100792480 (DE-599)DOAJe9f61abcfafa4e92872ba38af1d4f744 DE-627 ger DE-627 rakwb eng QB460-466 Bren E. Backhaus verfasserin aut CEERS Key Paper. VIII. Emission-line Ratios from NIRSpec and NIRCam Wide-Field Slitless Spectroscopy at z < 2 2024 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier We use James Webb Space Telescope Near-Infrared Camera Wide Field Slitless Spectroscopy (NIRCam WFSS) and the Near-Infrared spectrograph (NIRSpec) in the Cosmic Evolution Early Release survey to measure rest-frame optical emission-line ratios of 155 galaxies at z < 2. The blind NIRCam grism observations include a sample of galaxies with bright emission lines that were not observed on the NIRSpec masks. We study the changes of the H α , [O III ]/H β , and [Ne III ]/[O II ] emission lines in terms of redshift by comparing to lower-redshift SDSS, CLEAR, and MOSDEF samples. We find a significant (<3 σ ) correlation between [O III ]/H β with redshift, while [Ne III ]/[O II ] has a marginal (2 σ ) correlation with redshift. We compare [O III ]/H β and [Ne III ]/[O II ] to stellar mass and H β SFR. We find that both emission-line ratios have a correlation with H β SFR and an anticorrelation with stellar mass across the redshifts 0 < z < 9. Comparison with MAPPINGS V models indicates that these trends are consistent with lower metallicity and higher ionization in low-mass and high-SFR galaxies. We additionally compare to IllustrisTNG predictions and find that they effectively describe the highest [O III ]/H β ratios observed in our sample, without the need to invoke MAPPINGS models with significant shock ionization components. Emission line galaxies Galaxy evolution Galaxies Active galaxies Astrophysics Jonathan R. Trump verfasserin aut Nor Pirzkal verfasserin aut Guillermo Barro verfasserin aut Steven L. Finkelstein verfasserin aut Pablo Arrabal Haro verfasserin aut Raymond C. Simons verfasserin aut Jessica Wessner verfasserin aut Nikko J. Cleri verfasserin aut Micaela B. Bagley verfasserin aut Michaela Hirschmann verfasserin aut David C. Nicholls verfasserin aut Mark Dickinson verfasserin aut Jeyhan S. Kartaltepe verfasserin aut Casey Papovich verfasserin aut Dale D. Kocevski verfasserin aut Anton M. Koekemoer verfasserin aut Laura Bisigello verfasserin aut Anne E. Jaskot verfasserin aut Ray A. Lucas verfasserin aut Intae Jung verfasserin aut Stephen M. Wilkins verfasserin aut L. Y. Aaron Yung verfasserin aut Henry C. Ferguson verfasserin aut Adriano Fontana verfasserin aut Andrea Grazian verfasserin aut Norman A. Grogin verfasserin aut Lisa J. Kewley verfasserin aut Allison Kirkpatrick verfasserin aut Jennifer M. Lotz verfasserin aut Laura Pentericci verfasserin aut Pablo G. Pérez-González verfasserin aut Swara Ravindranath verfasserin aut Rachel S. Somerville verfasserin aut Guang Yang verfasserin aut Benne W. Holwerda verfasserin aut Peter Kurczynski verfasserin aut Nimish P. Hathi verfasserin aut Caitlin Rose verfasserin aut Kelcey Davis verfasserin aut In The Astrophysical Journal IOP Publishing, 2022 962(2024), 2, p 195 (DE-627)269019219 (DE-600)1473835-1 15384357 nnns volume:962 year:2024 number:2, p 195 https://doi.org/10.3847/1538-4357/ad1520 kostenfrei https://doaj.org/article/e9f61abcfafa4e92872ba38af1d4f744 kostenfrei https://doi.org/10.3847/1538-4357/ad1520 kostenfrei https://doaj.org/toc/1538-4357 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2014 GBV_ILN_2088 GBV_ILN_2522 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 962 2024 2, p 195
allfieldsSound	10.3847/1538-4357/ad1520 doi (DE-627)DOAJ100792480 (DE-599)DOAJe9f61abcfafa4e92872ba38af1d4f744 DE-627 ger DE-627 rakwb eng QB460-466 Bren E. Backhaus verfasserin aut CEERS Key Paper. VIII. Emission-line Ratios from NIRSpec and NIRCam Wide-Field Slitless Spectroscopy at z < 2 2024 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier We use James Webb Space Telescope Near-Infrared Camera Wide Field Slitless Spectroscopy (NIRCam WFSS) and the Near-Infrared spectrograph (NIRSpec) in the Cosmic Evolution Early Release survey to measure rest-frame optical emission-line ratios of 155 galaxies at z < 2. The blind NIRCam grism observations include a sample of galaxies with bright emission lines that were not observed on the NIRSpec masks. We study the changes of the H α , [O III ]/H β , and [Ne III ]/[O II ] emission lines in terms of redshift by comparing to lower-redshift SDSS, CLEAR, and MOSDEF samples. We find a significant (<3 σ ) correlation between [O III ]/H β with redshift, while [Ne III ]/[O II ] has a marginal (2 σ ) correlation with redshift. We compare [O III ]/H β and [Ne III ]/[O II ] to stellar mass and H β SFR. We find that both emission-line ratios have a correlation with H β SFR and an anticorrelation with stellar mass across the redshifts 0 < z < 9. Comparison with MAPPINGS V models indicates that these trends are consistent with lower metallicity and higher ionization in low-mass and high-SFR galaxies. We additionally compare to IllustrisTNG predictions and find that they effectively describe the highest [O III ]/H β ratios observed in our sample, without the need to invoke MAPPINGS models with significant shock ionization components. Emission line galaxies Galaxy evolution Galaxies Active galaxies Astrophysics Jonathan R. Trump verfasserin aut Nor Pirzkal verfasserin aut Guillermo Barro verfasserin aut Steven L. Finkelstein verfasserin aut Pablo Arrabal Haro verfasserin aut Raymond C. Simons verfasserin aut Jessica Wessner verfasserin aut Nikko J. Cleri verfasserin aut Micaela B. Bagley verfasserin aut Michaela Hirschmann verfasserin aut David C. Nicholls verfasserin aut Mark Dickinson verfasserin aut Jeyhan S. Kartaltepe verfasserin aut Casey Papovich verfasserin aut Dale D. Kocevski verfasserin aut Anton M. Koekemoer verfasserin aut Laura Bisigello verfasserin aut Anne E. Jaskot verfasserin aut Ray A. Lucas verfasserin aut Intae Jung verfasserin aut Stephen M. Wilkins verfasserin aut L. Y. Aaron Yung verfasserin aut Henry C. Ferguson verfasserin aut Adriano Fontana verfasserin aut Andrea Grazian verfasserin aut Norman A. Grogin verfasserin aut Lisa J. Kewley verfasserin aut Allison Kirkpatrick verfasserin aut Jennifer M. Lotz verfasserin aut Laura Pentericci verfasserin aut Pablo G. Pérez-González verfasserin aut Swara Ravindranath verfasserin aut Rachel S. Somerville verfasserin aut Guang Yang verfasserin aut Benne W. Holwerda verfasserin aut Peter Kurczynski verfasserin aut Nimish P. Hathi verfasserin aut Caitlin Rose verfasserin aut Kelcey Davis verfasserin aut In The Astrophysical Journal IOP Publishing, 2022 962(2024), 2, p 195 (DE-627)269019219 (DE-600)1473835-1 15384357 nnns volume:962 year:2024 number:2, p 195 https://doi.org/10.3847/1538-4357/ad1520 kostenfrei https://doaj.org/article/e9f61abcfafa4e92872ba38af1d4f744 kostenfrei https://doi.org/10.3847/1538-4357/ad1520 kostenfrei https://doaj.org/toc/1538-4357 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2014 GBV_ILN_2088 GBV_ILN_2522 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 962 2024 2, p 195
language	English
source	In The Astrophysical Journal 962(2024), 2, p 195 volume:962 year:2024 number:2, p 195
sourceStr	In The Astrophysical Journal 962(2024), 2, p 195 volume:962 year:2024 number:2, p 195
format_phy_str_mv	Article
institution	findex.gbv.de
topic_facet	Emission line galaxies Galaxy evolution Galaxies Active galaxies Astrophysics
isfreeaccess_bool	true
container_title	The Astrophysical Journal
authorswithroles_txt_mv	Bren E. Backhaus @@aut@@ Jonathan R. Trump @@aut@@ Nor Pirzkal @@aut@@ Guillermo Barro @@aut@@ Steven L. Finkelstein @@aut@@ Pablo Arrabal Haro @@aut@@ Raymond C. Simons @@aut@@ Jessica Wessner @@aut@@ Nikko J. Cleri @@aut@@ Micaela B. Bagley @@aut@@ Michaela Hirschmann @@aut@@ David C. Nicholls @@aut@@ Mark Dickinson @@aut@@ Jeyhan S. Kartaltepe @@aut@@ Casey Papovich @@aut@@ Dale D. Kocevski @@aut@@ Anton M. Koekemoer @@aut@@ Laura Bisigello @@aut@@ Anne E. Jaskot @@aut@@ Ray A. Lucas @@aut@@ Intae Jung @@aut@@ Stephen M. Wilkins @@aut@@ L. Y. Aaron Yung @@aut@@ Henry C. Ferguson @@aut@@ Adriano Fontana @@aut@@ Andrea Grazian @@aut@@ Norman A. Grogin @@aut@@ Lisa J. Kewley @@aut@@ Allison Kirkpatrick @@aut@@ Jennifer M. Lotz @@aut@@ Laura Pentericci @@aut@@ Pablo G. Pérez-González @@aut@@ Swara Ravindranath @@aut@@ Rachel S. Somerville @@aut@@ Guang Yang @@aut@@ Benne W. Holwerda @@aut@@ Peter Kurczynski @@aut@@ Nimish P. Hathi @@aut@@ Caitlin Rose @@aut@@ Kelcey Davis @@aut@@
publishDateDaySort_date	2024-01-01T00:00:00Z
hierarchy_top_id	269019219
id	DOAJ100792480
language_de	englisch
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callnumber-first	Q - Science
author	Bren E. Backhaus
spellingShingle	Bren E. Backhaus misc QB460-466 misc Emission line galaxies misc Galaxy evolution misc Galaxies misc Active galaxies misc Astrophysics CEERS Key Paper. VIII. Emission-line Ratios from NIRSpec and NIRCam Wide-Field Slitless Spectroscopy at z < 2
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topic_title	QB460-466 CEERS Key Paper. VIII. Emission-line Ratios from NIRSpec and NIRCam Wide-Field Slitless Spectroscopy at z < 2 Emission line galaxies Galaxy evolution Galaxies Active galaxies
topic	misc QB460-466 misc Emission line galaxies misc Galaxy evolution misc Galaxies misc Active galaxies misc Astrophysics
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title	CEERS Key Paper. VIII. Emission-line Ratios from NIRSpec and NIRCam Wide-Field Slitless Spectroscopy at z < 2
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title_full	CEERS Key Paper. VIII. Emission-line Ratios from NIRSpec and NIRCam Wide-Field Slitless Spectroscopy at z < 2
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author_browse	Bren E. Backhaus Jonathan R. Trump Nor Pirzkal Guillermo Barro Steven L. Finkelstein Pablo Arrabal Haro Raymond C. Simons Jessica Wessner Nikko J. Cleri Micaela B. Bagley Michaela Hirschmann David C. Nicholls Mark Dickinson Jeyhan S. Kartaltepe Casey Papovich Dale D. Kocevski Anton M. Koekemoer Laura Bisigello Anne E. Jaskot Ray A. Lucas Intae Jung Stephen M. Wilkins L. Y. Aaron Yung Henry C. Ferguson Adriano Fontana Andrea Grazian Norman A. Grogin Lisa J. Kewley Allison Kirkpatrick Jennifer M. Lotz Laura Pentericci Pablo G. Pérez-González Swara Ravindranath Rachel S. Somerville Guang Yang Benne W. Holwerda Peter Kurczynski Nimish P. Hathi Caitlin Rose Kelcey Davis
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title_sort	ceers key paper. viii. emission-line ratios from nirspec and nircam wide-field slitless spectroscopy at z < 2
callnumber	QB460-466
title_auth	CEERS Key Paper. VIII. Emission-line Ratios from NIRSpec and NIRCam Wide-Field Slitless Spectroscopy at z < 2
abstract	We use James Webb Space Telescope Near-Infrared Camera Wide Field Slitless Spectroscopy (NIRCam WFSS) and the Near-Infrared spectrograph (NIRSpec) in the Cosmic Evolution Early Release survey to measure rest-frame optical emission-line ratios of 155 galaxies at z < 2. The blind NIRCam grism observations include a sample of galaxies with bright emission lines that were not observed on the NIRSpec masks. We study the changes of the H α , [O III ]/H β , and [Ne III ]/[O II ] emission lines in terms of redshift by comparing to lower-redshift SDSS, CLEAR, and MOSDEF samples. We find a significant (<3 σ ) correlation between [O III ]/H β with redshift, while [Ne III ]/[O II ] has a marginal (2 σ ) correlation with redshift. We compare [O III ]/H β and [Ne III ]/[O II ] to stellar mass and H β SFR. We find that both emission-line ratios have a correlation with H β SFR and an anticorrelation with stellar mass across the redshifts 0 < z < 9. Comparison with MAPPINGS V models indicates that these trends are consistent with lower metallicity and higher ionization in low-mass and high-SFR galaxies. We additionally compare to IllustrisTNG predictions and find that they effectively describe the highest [O III ]/H β ratios observed in our sample, without the need to invoke MAPPINGS models with significant shock ionization components.
abstractGer	We use James Webb Space Telescope Near-Infrared Camera Wide Field Slitless Spectroscopy (NIRCam WFSS) and the Near-Infrared spectrograph (NIRSpec) in the Cosmic Evolution Early Release survey to measure rest-frame optical emission-line ratios of 155 galaxies at z < 2. The blind NIRCam grism observations include a sample of galaxies with bright emission lines that were not observed on the NIRSpec masks. We study the changes of the H α , [O III ]/H β , and [Ne III ]/[O II ] emission lines in terms of redshift by comparing to lower-redshift SDSS, CLEAR, and MOSDEF samples. We find a significant (<3 σ ) correlation between [O III ]/H β with redshift, while [Ne III ]/[O II ] has a marginal (2 σ ) correlation with redshift. We compare [O III ]/H β and [Ne III ]/[O II ] to stellar mass and H β SFR. We find that both emission-line ratios have a correlation with H β SFR and an anticorrelation with stellar mass across the redshifts 0 < z < 9. Comparison with MAPPINGS V models indicates that these trends are consistent with lower metallicity and higher ionization in low-mass and high-SFR galaxies. We additionally compare to IllustrisTNG predictions and find that they effectively describe the highest [O III ]/H β ratios observed in our sample, without the need to invoke MAPPINGS models with significant shock ionization components.
abstract_unstemmed	We use James Webb Space Telescope Near-Infrared Camera Wide Field Slitless Spectroscopy (NIRCam WFSS) and the Near-Infrared spectrograph (NIRSpec) in the Cosmic Evolution Early Release survey to measure rest-frame optical emission-line ratios of 155 galaxies at z < 2. The blind NIRCam grism observations include a sample of galaxies with bright emission lines that were not observed on the NIRSpec masks. We study the changes of the H α , [O III ]/H β , and [Ne III ]/[O II ] emission lines in terms of redshift by comparing to lower-redshift SDSS, CLEAR, and MOSDEF samples. We find a significant (<3 σ ) correlation between [O III ]/H β with redshift, while [Ne III ]/[O II ] has a marginal (2 σ ) correlation with redshift. We compare [O III ]/H β and [Ne III ]/[O II ] to stellar mass and H β SFR. We find that both emission-line ratios have a correlation with H β SFR and an anticorrelation with stellar mass across the redshifts 0 < z < 9. Comparison with MAPPINGS V models indicates that these trends are consistent with lower metallicity and higher ionization in low-mass and high-SFR galaxies. We additionally compare to IllustrisTNG predictions and find that they effectively describe the highest [O III ]/H β ratios observed in our sample, without the need to invoke MAPPINGS models with significant shock ionization components.
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container_issue	2, p 195
title_short	CEERS Key Paper. VIII. Emission-line Ratios from NIRSpec and NIRCam Wide-Field Slitless Spectroscopy at z < 2
url	https://doi.org/10.3847/1538-4357/ad1520 https://doaj.org/article/e9f61abcfafa4e92872ba38af1d4f744 https://doaj.org/toc/1538-4357
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up_date	2024-07-03T16:42:50.466Z
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fullrecord_marcxml	<?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>01000naa a22002652 4500</leader><controlfield tag="001">DOAJ100792480</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20240414125636.0</controlfield><controlfield tag="007">cr uuu---uuuuu</controlfield><controlfield tag="008">240414s2024 xx \|\|\|\|\|o 00\| \|\|eng c</controlfield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.3847/1538-4357/ad1520</subfield><subfield code="2">doi</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)DOAJ100792480</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-599)DOAJe9f61abcfafa4e92872ba38af1d4f744</subfield></datafield><datafield tag="040" ind1=" " ind2=" "><subfield code="a">DE-627</subfield><subfield code="b">ger</subfield><subfield code="c">DE-627</subfield><subfield code="e">rakwb</subfield></datafield><datafield tag="041" ind1=" " ind2=" "><subfield code="a">eng</subfield></datafield><datafield tag="050" ind1=" " ind2="0"><subfield code="a">QB460-466</subfield></datafield><datafield tag="100" ind1="0" ind2=" "><subfield code="a">Bren E. Backhaus</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">CEERS Key Paper. VIII. Emission-line Ratios from NIRSpec and NIRCam Wide-Field Slitless Spectroscopy at z < 2</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">2024</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="a">Text</subfield><subfield code="b">txt</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="a">Computermedien</subfield><subfield code="b">c</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="a">Online-Ressource</subfield><subfield code="b">cr</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">We use James Webb Space Telescope Near-Infrared Camera Wide Field Slitless Spectroscopy (NIRCam WFSS) and the Near-Infrared spectrograph (NIRSpec) in the Cosmic Evolution Early Release survey to measure rest-frame optical emission-line ratios of 155 galaxies at z < 2. The blind NIRCam grism observations include a sample of galaxies with bright emission lines that were not observed on the NIRSpec masks. We study the changes of the H α , [O III ]/H β , and [Ne III ]/[O II ] emission lines in terms of redshift by comparing to lower-redshift SDSS, CLEAR, and MOSDEF samples. We find a significant (<3 σ ) correlation between [O III ]/H β with redshift, while [Ne III ]/[O II ] has a marginal (2 σ ) correlation with redshift. We compare [O III ]/H β and [Ne III ]/[O II ] to stellar mass and H β SFR. We find that both emission-line ratios have a correlation with H β SFR and an anticorrelation with stellar mass across the redshifts 0 < z < 9. Comparison with MAPPINGS V models indicates that these trends are consistent with lower metallicity and higher ionization in low-mass and high-SFR galaxies. 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CEERS Key Paper. VIII. Emission-line Ratios from NIRSpec and NIRCam Wide-Field Slitless Spectroscopy at z < 2

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